Abstract
Observations of the surface abundances of lithium, beryllium and helium-3 in the Sun and in solar-type stars of different ages should be interpreted in a coherent way. The abundance of lithium at the surface of a star decreases slowly with age; for stars of the same age it decreases with mass and a dependence on the rotation velocity is suggested. The solar surface lithium is depleted by a factor of 100 relative to the cosmic abundance while an He-3 enrichment of 15% at the solar surface during evolution is suggested.
Observations favour the hypothesis of a slow transport process at work between the outer convective zone and the radiative interior of these stars. Orders of magnitude of the transport coefficient as well as its dependence upon the physical parameters can be inferred from surface abundances of light elements, but at the moment we are far from producing a completely consistent modelization.
Access this chapter
Tax calculation will be finalised at checkout
Purchases are for personal use only
Preview
Unable to display preview. Download preview PDF.
References
Baglin, A., Morel, P. J. 1983, in Observational Tests of the Stellar Evolution Theory, IAU Symp. No. 105, eds A. Maeder, A. Renzini, Reidel Dordrecht 1984, p. 529
Baglin, A., Morel, P.J., Schatzman, E. 1985, Astron. Astrophys. 149, 309
Baglin, A., Morel P.J. 1987, in the Impact of Very High SIN Spectroscopy on Stellar Physics, IAU Symp. No. 132, eds G. Cayrel and M. Spite, Kluwer Academic Publishers 1988, p. 279.
Baglin, A., Morel P.J. 1989, in preparation
Balachandran, S., Lambert, D.L., Stauffer, J.R. 1988, Astrophys. J. 333, 267
Bodenheimer, P. 1965, Astrophys. J. 142, 451
Boesgaard, A.M. 1976, Publ. Astron. Soc. Pacific 88, 353
Boesgaard, A.M. 1987, Astrophys. J., 321, 967
Boesgaard, A.M., Budge, K.B., Burck, E.E. 1988a, Astrophys. J. 325, 749
Boesgaard, A.M., Budge, K.B., Ramsay, M.A. 1988b, Astrophys. J. 327, 389
Boesgaard, A.M., Tripicco M.J. 1986a, Astrophys. J. 302, L49
Boesgaard, A.M., Tripicco M.J. 1986b, Astrophys. J. 303, 724
Bochsler, P., Geiss, J., Maeder, A. 1989, in Inside the Sun, Proc. IAU Colloquium 121, Versailles, France 22–26 May 1989, to be published in Solar Physics
Butler, R.P., Cohen, R.D., Duncan, D.K., Marcy, G.W. 1987, Astrophys. J. 319, L19
Caughlan, G.R., Fowler, W.A. 1988, Atomic Data and Nucl. Data Tables 40, 283
Cayrel, R. 1983, in Observational Tests of the Stellar Evolution Theory, IAU Symp. No. 105, eds A. Maeder, A. Renzini, Reidel Dordrecht 1984, p. 533.
Cayrel, R., Cayrel de Strobel, G., Campbell, B., Däppen W. 1984, Astrophys. J. 283, 205
Cayrel de Strobel, G., Spite, M. 1987, eds. of IAU Symp. No. 132 on the Impact of Very High SIN Spectroscopy on Stellar Physics, Kluwer Academic Publishers 1988.
Cayrel R., Cayrel de Strobel G., Bentolila C. 1989 in preparation.
Conti, P.S. 1968, Astrophys. J. 152, 657
D’Antona, F., Mazzitelli I. 1984, Astron. Astrophys. 138, 431
Danziger, I.J. 1967, Astrophys. J. 150, 733
Danziger, I.J., Conti P.S. 1966, Astrophys. J. 146, 392
Duncan, D.K., Jones, B.F. 1983, Astrophys. J. 271, 663
Garcia Lopez, R.J., Rebolo, R., Beckman, J.E. 1988, Publ. Astron. Soc. Pacific100, 1489
Geiss J. 1971, in Solar Wind, NASA SP-308, p. 559
Herbig, G.H. 1965, Astrophys. J. 141, 588
Hobbs, L.M., Pilachowski, C. 1986a, Astrophys. J. 309, L17 - L21
Hobbs, L.M., Pilachowski, C. 1986b, Astrophys. J. 311, L37 - L40
Kraft, R.P., Wilson, O.C. 1965, Astrophys. J. 141, 828
Lebreton, Y., Maeder, A. 1986, Astron. Astrophys. 161, 119
Lebreton, Y., Maeder A. 1987, Astron. Astrophys. 175, 99
Nichiporuk W., Moore C.B. 1974, Geoch. Cosmoch. Acta 38, 1691
Pinsonneault, M.H., Kawaler, S.D., Sofia, S., Demarque, P. 1989, Astrophys. J. 338, 424
Rebolo, R., Beckman, J.E. 1988, Astron. Astrophys. 201, 267
Schatzman E., 1969, Astron. Astrophys. 3, 339
Schatzman E., 1981, in Turbulent diffusion and the solar neutrino problem, CERN 81–11 Schatzman E. 1989, in preparation
Soderblom, DR., Stauffer, J.R. 1984, Astronom. J. 89. 1543
Spite, F., Spite, M., Peterson, R.C., Chaffee, F.H. Jr.: 1987, Astron. Astrophys. 171, L8
Stauffer, J. 1987, in Cool Stars, stellar systems ans the sun. Proceedings of the fifth Cambridge Workshop,Boulder, p; 182.
Straus, J.M., Blake, J.B., Schramm, D.N. 1976, Astrophys. J. 204, 481
Vauclair, S. 1988, Astrophys. J. 335, 971
Wallerstein, G., Herbig, G.H., Conti, P.S. 1965, Astrophys. J. 141, 610
Weymann, R., Sears, R.L. 1965, Astrophys. J. 142, 174
Zahn, J.P. 1983, in Astrophysical Processes in Upper Main Sequence Stars, 13th Advanced Course SaasFee, Publ. Geneva Observatory
Zahn, J.P. 1987, in The internal angular velocity of the Sun eds; B.R. Dumey and S. Sofia, Reidel, Dordrecht, p. 201.
Zappala, R.R. 1972, Astrophys. J. 172, 57
Author information
Authors and Affiliations
Editor information
Editors and Affiliations
Rights and permissions
Copyright information
© 1990 Kluwer Academic Publishers
About this paper
Cite this paper
Baglin, A., Lebreton, Y. (1990). Surface Abundances of Light Elements as Diagnostics of Transport Processes in the Sun and Solar-Type Stars. In: Berthomieu, G., Cribier, M. (eds) Inside the Sun. Astrophysics and Space Science Library, vol 159. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-0541-2_36
Download citation
DOI: https://doi.org/10.1007/978-94-009-0541-2_36
Publisher Name: Springer, Dordrecht
Print ISBN: 978-94-010-6730-0
Online ISBN: 978-94-009-0541-2
eBook Packages: Springer Book Archive